Alternative formulations of the thermodynamics of scalar-tensor theories

被引:0
|
作者
Gallerani, Luca [1 ,2 ]
Miranda, Marcello [3 ,4 ]
Giusti, Andrea [1 ,5 ]
Mentrelli, Andrea [1 ,2 ,6 ]
机构
[1] Alma Mater Res Ctr Appl Math AM 2, Via Saragozza 8, I-40123 Bologna, Italy
[2] Univ Bologna, Dept Math, Piazza Porta San Donato 5, I-40126 Bologna, Italy
[3] Scuola Super Meridionale, Largo San Marcellino 10, I-80138 Naples, Italy
[4] Complesso Univ Monte Sant Angelo, Ist Nazl Fis Nucleare, Sez Napoli, Edificio G,Via Cinthia, I-80126 Naples, Italy
[5] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, England
[6] Ist Nazl Fis Nucleare INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy
基金
英国科学技术设施理事会;
关键词
BLACK-HOLES;
D O I
10.1103/PhysRevD.110.064087
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We explore alternative formulations of the analogy between viable Horndeski gravity and Eckart's first-order thermodynamics. We single out a class of identifications for the effective stress-energy tensor of the scalar field fluid that, upon performing the imperfect fluid decomposition, yields constitutive relations that can be mapped onto Eckart's theory. We then investigate how different couplings to Einstein's gravity, at the level of the field equations, can affect the thermodynamic formalism overall. Last, we specialize the discussion to the case of "traditional" scalar-tensor theories and identify a specific choice of the coupling function that leads to a significant simplification of the formalism.
引用
收藏
页数:8
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